Showing 1–20 of 46 results
/ Date/ Name
Jan 28, 2026Performance of the Particle-Identification Silicon-Telescope Array Coupled with the VAMOS++ Magnetic SpectrometerJan 26, 2026Level structure of light neutron-rich La isotopes beyond the N=82 shell closureDec 12, 2025JWST/NIRSpec Detects Warm CO Emission in the Terrestrial-Planet Zone of HD 131488Sep 22, 2025Technical overview and architecture of the FastNet Machine Learning weather prediction model, version 1.0Sep 22, 2025FastNet: Improving the physical consistency of machine-learning weather prediction models through loss function designMay 16, 2025Unbound neutron $\nu0d_{3/2}$ strength in $^{17}$C and the N=16 shell gapApr 7, 2025The UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Large Director's Discretionary Program with Hubble. I. Goals, Design, and Initial ResultsNov 11, 2024The Mega-MUSCLES Treasury Survey: X-ray to infrared Spectral Energy Distributions of a representative sample of M dwarfsJun 28, 2024High-energy spectra of LTT 1445A and GJ 486 reveal flares and activityMay 24, 2024High-resolution spectroscopy of neutron-rich Br isotopes and signatures for a prolate-to-oblate shape transition at N=56Nov 13, 2023CATLIFE (Complementary Arm for Target LIke FragmEnts): Spectrometer for Target like fragments at VAMOS++Nov 13, 2023Particle Identification at VAMOS++ with Machine Learning TechniquesJun 23, 2023Characterising a World Within the Hot Neptune Desert: Transit Observations of LTT 9779 b with HST WFC3Feb 16, 2023Cross-shell states in $^{15}$C: a test for p-sd interactionsAug 24, 2022Identification of carbon dioxide in an exoplanet atmosphereApr 21, 2021Neutron-proton pairing in the N=Z radioactive fp-shell nuclei 56Ni and 52Fe probed by pair transferMar 23, 2021PENELLOPE: the ESO data legacy program to complement the Hubble UV Legacy Library of Young Stars (ULLYSES) I. Survey presentation and accretion properties of Orion OB1 and $σ$-OrionisFeb 22, 2021The Mega-MUSCLES Spectral Energy Distribution Of TRAPPIST-1Feb 16, 2021Reconstructing the Extreme Ultraviolet Emission of Cool Dwarfs Using Differential Emission Measure PolynomialsNov 11, 2020Low-lying single-particle structure of 17C and the N = 14 sub-shell closure